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Period decrease in three SuperWASP eclipsing binary candidates near the short-period limit

Lohr, M. E.; Norton, A. J.; Kolb, U. C.; Anderson, D. R.; Faedi, F. and West, R. G. (2012). Period decrease in three SuperWASP eclipsing binary candidates near the short-period limit. Astronomy & Astrophysics, 542, article no. A124.

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SuperWASP light curves for 53 W UMa-type eclipsing binary (EB) candidates, identified in previous work as being close to the contact binary short-period limit, were studied for evidence of period change. The orbital periods of most of the stars were confirmed, and period decrease, significant at more than 5σ, was observed in three objects: 1SWASPJ174310.98+432709.6 (-0.055 ± 0.003 s yr-1), 1SWASPJ133105.91+121538.0 (-0.075 ± 0.013 s yr-1) and 1SWASPJ234401.81-212229.1 (-0.313 ± 0.019 s yr-1). The magnitudes of the observed period changes cannot be explained by magnetic braking or gravitational radiation effects, and are most likely primarily due to unstable mass transfer from primary to secondary components, possibly accompanied by unstable mass and angular momentum loss from the systems. If these period decreases persist, the systems could merge on a relatively short timescale.

Item Type: Journal Item
Copyright Holders: 2012 ESO
ISSN: 1432-0746
Project Funding Details:
Funded Project NameProject IDFunding Body
Not SetNot SetSTFC (Science & Technology Facilities Council)
Not SetNot SetThe Open University (OU)
Extra Information: 6 pp.
Keywords: variable stars; binaries; V1067Her; GSC 2314-0530
Academic Unit/School: Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
Item ID: 33879
Depositing User: Andrew Norton
Date Deposited: 20 Jun 2012 12:16
Last Modified: 07 Dec 2018 16:32
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